1. Rapid Response of Martian Magnetotail to Solar Wind Disturbance: Tianwen‐1 and MAVEN Joint Observations.
- Author
-
Guo, Z. Z., Fu, H. S., Cao, J. B., Wang, Y. M., Ge, M., Zhou, T. Y., Fu, W. D., and Wang, Z.
- Subjects
INTERPLANETARY magnetic fields ,SOLAR magnetic fields ,DYNAMIC pressure ,MARTIAN atmosphere ,MAGNETOSPHERE ,IONOSPHERE ,SOLAR wind - Abstract
The Martian magnetotail is largely controlled by the solar wind (SW) and is modulated by variations in the upstream drivers. However, due to the limitations of single‐spacecraft observations, the effects of SW variations on the Martian magnetotail have not been fully understood so far. Here, using Tianwen‐1 and MAVEN data, we report for the first time the rapid response of Martian magnetotail to the SW disturbance. In our study, Tianwen‐1 detected the flapping of Martian magnetotail, while MAVEN monitored disturbances in the upstream SW. The results indicate that a 20% increase (or decrease) in SW dynamic pressure and a 30° (or 50°) rotation of interplanetary magnetic field clock angle could cause the Martian magnetotail to swing rapidly. These two SW disturbances could lead to oscillations of the Martian magnetotail. This study reveals the importance of joint observations for studying the interaction between the SW and Mars. Plain Language Summary: Mars lacks an intrinsic global magnetic field and as a result solar wind (SW) interacts directly with its ionosphere and atmosphere, leading to a high dependence of the Martian induced magnetosphere on SW conditions. Understanding the interaction between the SW and Mars can provide critical information for studies of planetary evolution, especially the effect of the SW on the Martian magnetotail. In previous studies, using single satellite observations, we limit ourselves to studying some local physical processes or statistical properties. Here, based on the joint measurements by Tianwen‐1 and MAVEN, we observed the rapid response of Martian magnetotail to the SW disturbance, finding that a 20% increase (or decrease) in SW dynamic pressure and a 30° (or 50°) rotation of IMF clock angle could cause the Martian magnetotail to swing rapidly. These two SW disturbances could lead to oscillations of the Martian magnetotail. These results can help us understand the SW interaction with the Martian induced magnetosphere. Key Points: We report for the first time the rapid response of Martian magnetotail to the solar wind (SW) disturbance by using Tianwen‐1 and MAVEN dataA 20% increase (or decrease) in PSW and a 30° (or 50°) rotation of interplanetary magnetic field clock angle could cause the Martian magnetotail to swingThese two SW disturbances could lead to oscillations of the Martian magnetotail [ABSTRACT FROM AUTHOR]
- Published
- 2024
- Full Text
- View/download PDF